Constraints on muon-specific dark forces

Savely G. Karshenboim, David McKeen, and Maxim Pospelov
Phys. Rev. D 90, 073004 – Published 13 October 2014; Erratum Phys. Rev. D 90, 079905 (2014)

Abstract

The recent measurement of the Lamb shift in muonic hydrogen allows for the most precise extraction of the charge radius of the proton which is currently in conflict with other determinations based on ep scattering and hydrogen spectroscopy. This discrepancy could be the result of some new muon-specific force with O(1–100) MeV force carrier—in this paper we concentrate on vector mediators. Such an explanation faces challenges from the constraints imposed by the g2 of the muon and electron as well as precision spectroscopy of muonic atoms. In this work we complement the family of constraints by calculating the contribution of hypothetical forces to the muonium hyperfine structure. We also compute the two-loop contribution to the electron parity-violating amplitude due to a muon loop, which is sensitive to the muon axial-vector coupling. Overall, we find that the combination of low-energy constraints favors the mass of the mediator to be below 10 MeV and that a certain degree of tuning is required between vector and axial-vector couplings of new vector particles to muons in order to satisfy constraints from muon g2. However, we also observe that in the absence of a consistent standard model embedding high-energy weak-charged processes accompanied by the emission of new vector particles are strongly enhanced by (E/mV)2, with E a characteristic energy scale and mV the mass of the mediator. In particular, leptonic W decays impose the strongest constraints on such models completely disfavoring the remainder of the parameter space.

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  • Received 31 August 2014
  • Publisher error corrected 16 October 2014

DOI:https://doi.org/10.1103/PhysRevD.90.073004

© 2014 American Physical Society

Corrections

16 October 2014

Erratum

Publisher’s Note: Constraints on muon-specific dark forces [Phys. Rev. D 90, 073004 (2014)]

Savely G. Karshenboim, David McKeen, and Maxim Pospelov
Phys. Rev. D 90, 079905 (2014)

Authors & Affiliations

Savely G. Karshenboim1,2, David McKeen3, and Maxim Pospelov4,5

  • 1Max-Planck-Institut für Quantenoptik, Garching 85748, Germany
  • 2Pulkovo Observatory, St. Petersburg, 196140, Russia
  • 3Department of Physics, University of Washington, Seattle, Washington 98195, USA
  • 4Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8P 5C2, Canada
  • 5Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2J 2W9, Canada

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Issue

Vol. 90, Iss. 7 — 1 October 2014

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